Planned stereo pairs have suitable stereo convergence angles and illumination by design.
In addition to planned stereo pairs, the Pairendipity software can identify overlapping
HiRISE images that are serendipitously suitable for stereo processing and find stereo
pairs within the CTX dataset.
Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below.
Since this list is based on produced stereo anaglyphs it also contains a few serendipitous
pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed
in the “Pairendipity Stereo” link, while CTX stereo pairs are listed
in “Pairendipity CTX Stereo”.
Images taken close together in time minimize illumination and frost differences and are
especially useful (see the Delta-Days column in the Pairendipity files or difference
the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs
with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.
| Exposure of North Polar Layered Deposits: ESP_089303_2605 ESP_089962_2605 (Interval in Earth days: 52) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.27 | 345. | 0.31 | 14.90 | 62.1 | 69.6 |
| Mamers Valles: ESP_089329_2175 ESP_089606_2175 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 37.21 | 13.9 | -10. | -29.1 | 48.8 | 52.9 |
| Thermal Anomaly in Young Lava Flows of Elysium Region: ESP_089284_1970 ESP_089429_1970 (Interval in Earth days: 11) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 17.03 | 163. | 2.69 | 16.88 | 49.6 | 48.9 |
| Potential Compound Dune: ESP_089573_2610 ESP_089389_2610 (Interval in Earth days: 14) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 80.87 | 160. | 19.2 | -5.86 | 64.3 | 63.7 |
| Possible Sulfate-Rich Deposit: ESP_089319_1730 ESP_089741_1730 (Interval in Earth days: 32) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -7.16 | 291. | 5.45 | -5.79 | 59.4 | 59.6 |
| Possible Vent in Young Lava Flows in Elysium Region: ESP_089244_2090 ESP_089534_2090 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 28.68 | 174. | 4.31 | 28.13 | 47.1 | 46.6 |
| Sample of Scalloped Terrain West of Erebus Montes: ESP_089349_2195 ESP_089072_2195 (Interval in Earth days: 22) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.37 | 187. | -8.3 | 14.20 | 48.9 | 44.9 |
| Large Crater on Slope of Layered Deposits: ESP_089517_1735 ESP_089095_1735 (Interval in Earth days: 33) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -6.23 | 287. | -20. | -5.59 | 60.6 | 59.8 |
| Features around Crater in Terra Sabaea: ESP_089319_2205 ESP_089385_2205 (Interval in Earth days: 5) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | 39.93 | 284. | 8.56 | -7.88 | 47.1 | 49.1 |
| Light-Toned Deposits in Iani Chaos: ESP_089383_1780 ESP_089871_1780 (Interval in Earth days: 38) | Center lat. | Center long. | 1st half roll angle | 2nd half roll angle | 1st half incidence angle | 2nd half incidence angle | -1.75 | 341. | 18.5 | -11.7 | 55.6 | 57.9 |
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